1. Chengao Liu, Xinhua Zhao1, Tao Chen, Huichao Li, Predicting short-term F10.7 with transportmodels, Astrophys Space Sci(2018) 363:266, https://doi.org/10.1007/s10509-018-3476-x. [pdf]

2. ZHAO Xinhua, ZHANG Min, WANG Yuming, HE Jiansen, NING Hao, QIN Gang, Interplanetary physics in Mainland China, Chin. J. Space Sci., 2018, 385 665-693, doi: 10.11728/cjss2018.05.665. [pdf]

3. Zehao Wang, Jianpeng Guo, Xueshang Feng, Chaoxu Liu, Hui Huang, Haibo Lin, Chenming Tan, Yihua Yan, and Weixing Wan, The Merging of Two Stream Interaction Regions within 1 au The Possible Role of Magnetic Reconnection, The Astrophysical Journal Letters, 869, L6, 2018, https://doi.org/10.3847/2041-8213/aaf398.. [pdf]

4. Man Zhang, Yu Fen Zhou, Xue Shang Feng1, Bo Li, and Ming Xiong, Numerical study of the reconnection process between magnetic cloud and heliospheric current sheet, A&A 619, A82 2018，https://doi.org/10.1051/0004-6361/201832951.[pdf]

5. Keiji Hayashi, Xueshang Feng, Ming Xiong, Chaowei Jiang, Erratum: “An MHD Simulation of Solar Active Region 11158 Driven with Timedependent Electric Field Determined from HMI Vector Magnetic Field Measurement Data”, Astrophys. J., 2018, 856, 181. [pdf]

6. Ming Xiong, Jackie A. Davies, Xueshang Feng, Bo Li, Liping Yang, Lidong Xia, Richard A. Harrison, Keiji Hayashi, Huichao Li, and Yufen Zhou, Prospective White-light Imaging and In Situ Measurements of Quiescent Large-scale Solar-wind Streams from the Parker Solar Probe and Solar Orbiter, The Astrophysical Journal, 868:137(17pp), 2018, http://iopscience.iop.org/article/10.3847/1538-4357/aae978/pdf. [pdf]

7. Wenwen Wei, Fang Shen, Zicai Yang, Lulu Zhao, Yang Wang, Pingbing Zuo and Jie Zhang, Modeling solar energetic particle transport in 3D background solar wind Influences of the compression regions, Journal of Atmospheric and Solar-Terrestrial Physics, 1822019 155-164, https://doi.org/10.1016/j.jastp.2018.11.012.

8. 杨子才，沈芳，杨易，冯学尚, WSA太阳风经验模型及其应用, 空间科学学报，2018, 38(3):285-295, doi: 10.11728/cjss2018.03.285. [pdf]

9. 杨子才，沈芳，杨易等, 行星际背景太阳风的三维MHD数值模拟, 地球物理学报，61(11):4337-4347, doi: 0.6038/cjg2018l0515. [pdf]

10. Yuan Wang, Xueshang Feng, Changqing Xiang, An effective matrix-free implicit scheme for the magnetohydrodynamic solar wind simulations, Computers and Fluids 179 2018 67–77, https://doi.org/10.1016/j.compfluid.2018.10.014. [pdf]

11. Yun Yang, Xue-Shang Feng, Chao-Wei Jiang, and Ward B. Manchester, A study of the emergence of flux rope from the solar convection zone into the atmosphere by using a novel numerical method, Physics of Plasmas 25, 090702 2018, doi: 10.1063/1.5044646.

12. Caixia Li, Xueshang Feng, Changqing Xiang, Man Zhang, Huichao Li, and Fengsi Wei, Solar Coronal Modeling by Path-conservative HLLEM Riemann Solver, 2018 ApJ 867 42, doi: 10.3847/1538-4357/aae200. [pdf]

13. Liping Yang and Lei Zhang and Jiansen He and Chuanyi Tu and Shengtai Li and Xin Wang and Linghua Wang, Coexistence of Slow-mode and Alfvén-mode Waves and Structures in 3D Compressive MHD Turbulence, The Astrophysical Journal, 8661, 41, 2018，http://stacks.iop.org/0004-637X/866/i=1/a=41. [pdf]

14. Fang Shen, Zicai Yang, Jie Zhang, Wenwen Wei and Xueshang Feng 2018, Three-dimensional MHD Simulation of Solar Wind Using a New Boundary Treatment Comparison with In Situ Data at Earth, Astrophys. J., 866, 18 15pp. https://doi.org/10.3847/1538-4357/aad806. [pdf]

15. Zilu Zhou, Fengsi Wei, Xueshang Feng, Yi Wang, Pingbing Zuo, and Xiaojun Xu, Observation of Interplanetary Slow Shock Pair Associated with Reconnection Exhaust in Magnetic Cloud Boundary Layer, The Astrophysical Journal, 86384 7pp, 2018 https://doi.org/10.3847/1538-4357/aad098. [pdf]

16. Yun Yang, Xue-ShangFeng, Chao-Wei Jiang, An upwind CESE scheme for 2D and 3D MHD numerical simulation in general curvilinear coordinates, Journal of Computational Physics 3712018 850–869   https://doi.org/10.1016/j.jcp.2018.05.014. [pdf]

17. Lei Zhang, Jiansen He, Jinsong Zhao, Shuo Yao, and Xueshang Feng, Nature of Magnetic Holes above Ion Scales A Mixture of Stable Slow Magnetosonic and Unstable Mirror Modes in a Double-polytropic Scenario?, The Astrophysical Journal, 86435 8pp, 2018  https://doi.org/10.3847/1538-4357/aad4aa. [pdf]

18. Xi Luo, Marius S. Potgieter, Ming Zhang , and Xueshang Feng, A Study of Electron Forbush Decreases with a 3D SDE Numerical Model, The Astrophysical Journal, 860160 9pp, 2018 https://doi.org/10.3847/1538-4357/aac5f2. [pdf]

19. Yang, Y., Shen, F., Yang, Z., & Feng, X.(2018), Prediction of Solar Wind Speed at 1 AU Using an Artificial Neural Network, Space Weather, 16, doi: 10.1029/2018SW001955. [pdf]

20. Yudong Ye and M.B. Korsós and R. Erdélyi, Detailed analysis of dynamic evolution of three Active Regions at the photospheric level before flare and CME occurrence, Advances in Space Research, 61(2), 673 - 682, 2018. [pdf]

21. Huichao Li，Xueshang Feng, CESE‐HLL Magnetic Field Driven Modeling of the Background Solar Wind During Year 2008, Journal ofgeophysical Research Space physics, 2018, https//doi.org/10.1029/2017JA025125.

22. Liping Yang等, Disappearance of Anisotropic Intermittency in Large-amplitude MHD Turbulence and Its Comparison with Small-amplitude MHD Turbulence, The Astrophysical Journal, 85569 9pp, 2018.

23. Keiji Hayashi, Xueshang Feng, Ming Xiong, Chaowei Jiang, An MHD Simulation of Solar Active Region 11158 Driven with a Time-dependent Electric Field Determined from HMI Vector Magnetic Field Measurement Data, Astrophys. J., 2018, 85511. [pdf]

24. Liping Yang等, Formation of Cool and Warm Jets by Magnetic Flux Emerging from the Solar Chromosphere to Transition Region, The Astrophysical Journal, 85216 15pp, 2018.

25. Zicai Yang， Fang Shen， Jie Zhang等, Correlation Between the Magnetic Field and Plasma Parameters at 1 AU, Solar Phys 2018 29324.

26. Paul S Cally, Ming Xiong, Sensitivity of coronal loop sausage mode frequencies and decay rates to radial and longitudinal density inhomogeneities: a spectral approach, Journal of Physics A: Mathematical and Theoretical, 2018, 51, 025501.[pdf]

27. Ming Xiong, Jackie A. Davies, Richard A. Harrison, Yufen Zhou, Xueshang Feng, et al., Prospective Out-of-ecliptic White-light Imaging of Coronal Mass Ejections Traveling through the Corona and Heliosphere, Astrophys. J., 2018, 852:111. [pdf]